{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:UN5GWKKK4VL4M5Z2P5ILGTBJVJ","short_pith_number":"pith:UN5GWKKK","schema_version":"1.0","canonical_sha256":"a37a6b294ae557c6773a7f50b34c29aa48d2fe71ac6de99e0b56d9e00070ff3d","source":{"kind":"arxiv","id":"0802.0758","version":1},"attestation_state":"computed","paper":{"title":"Dissipative structures of diffuse molecular gas III -- Small-scale intermittency of intense velocity-shears","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Edith Falgarone (LERMA), Jerome Pety (IRAM, LAOG), LERMA), Pierre Hily-Blant (IRAM","submitted_at":"2008-02-06T09:02:54Z","abstract_excerpt":"We further characterize the structures tentatively identified on thermal and chemical grounds as the sites of dissipation of turbulence in molecular clouds (Papers I and II). Our study is based on two-point statistics of line centroid velocities (CV), computed from three large 12CO maps of two fields. Probability density functions (PDF) of the CO line centroid velocity increments (CVI) over lags varying by an order of magnitude and structure functions of the line CV, up to the 6th order, are computed. We show that the line CV bear the three signatures of intermittency in a turbulent velocity f"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"0802.0758","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2008-02-06T09:02:54Z","cross_cats_sorted":[],"title_canon_sha256":"dae337159a4a5320b15a507017335e3c7497d5a08a16746ed2ecfcbcd5b192ec","abstract_canon_sha256":"c2357db732610274b891b82b29a1faab244ed315b04719fcb474c5cce096a31f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:09:11.054426Z","signature_b64":"0B6xmS1Tz1F3oIiqFrgwgwyH9nzAZhlUze9EML2asaz/piBg8xqRViO87eGm94/bly1uw7gqneJDGrGpko7ADg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a37a6b294ae557c6773a7f50b34c29aa48d2fe71ac6de99e0b56d9e00070ff3d","last_reissued_at":"2026-07-04T17:09:11.054056Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:09:11.054056Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dissipative structures of diffuse molecular gas III -- Small-scale intermittency of intense velocity-shears","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Edith Falgarone (LERMA), Jerome Pety (IRAM, LAOG), LERMA), Pierre Hily-Blant (IRAM","submitted_at":"2008-02-06T09:02:54Z","abstract_excerpt":"We further characterize the structures tentatively identified on thermal and chemical grounds as the sites of dissipation of turbulence in molecular clouds (Papers I and II). Our study is based on two-point statistics of line centroid velocities (CV), computed from three large 12CO maps of two fields. Probability density functions (PDF) of the CO line centroid velocity increments (CVI) over lags varying by an order of magnitude and structure functions of the line CV, up to the 6th order, are computed. We show that the line CV bear the three signatures of intermittency in a turbulent velocity f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0802.0758","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/0802.0758/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"0802.0758","created_at":"2026-07-04T17:09:11.054112+00:00"},{"alias_kind":"arxiv_version","alias_value":"0802.0758v1","created_at":"2026-07-04T17:09:11.054112+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0802.0758","created_at":"2026-07-04T17:09:11.054112+00:00"},{"alias_kind":"pith_short_12","alias_value":"UN5GWKKK4VL4","created_at":"2026-07-04T17:09:11.054112+00:00"},{"alias_kind":"pith_short_16","alias_value":"UN5GWKKK4VL4M5Z2","created_at":"2026-07-04T17:09:11.054112+00:00"},{"alias_kind":"pith_short_8","alias_value":"UN5GWKKK","created_at":"2026-07-04T17:09:11.054112+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21672","citing_title":"Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas","ref_index":224,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ","json":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ.json","graph_json":"https://pith.science/api/pith-number/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/graph.json","events_json":"https://pith.science/api/pith-number/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/events.json","paper":"https://pith.science/paper/UN5GWKKK"},"agent_actions":{"view_html":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ","download_json":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ.json","view_paper":"https://pith.science/paper/UN5GWKKK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0802.0758&json=true","fetch_graph":"https://pith.science/api/pith-number/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/graph.json","fetch_events":"https://pith.science/api/pith-number/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/action/storage_attestation","attest_author":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/action/author_attestation","sign_citation":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/action/citation_signature","submit_replication":"https://pith.science/pith/UN5GWKKK4VL4M5Z2P5ILGTBJVJ/action/replication_record"}},"created_at":"2026-07-04T17:09:11.054112+00:00","updated_at":"2026-07-04T17:09:11.054112+00:00"}